Black Hole – Moving Mirror I: An Exact Correspondence

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dc.contributor.authorPaul R. Anderson; Michael R.R. Good; Charles R. Evans
dc.date.accessioned2025-08-06T09:44:19Z
dc.date.available2025-08-06T09:44:19Z
dc.date.issued2018
dc.description.abstractAn exact correspondence is demonstrated between a specific moving mirror trajectory in 1+1D flat spacetime and a spacetime model in 1+1D describing black hole formation from a null-shell collapse. It is shown that the Bogolubov coefficients connecting “in” and “out” states are identical in both cases and the exact expressions are provided. A generalization to (3+1)D black hole spacetimes is discussed.
dc.identifier.citationAnderson, P. R., Good, M. R. R., & Evans, C. R. (2015). Black Hole – Moving Mirror I: An Exact Correspondence. In MG14: Proceedings of the Fourteenth Marcel Grossmann Meeting (World Scientific, 2018). arXiv:1507.03489 [gr-qc]. DOI: 10.1142/9789813226609_0171
dc.identifier.urihttps://nur.nu.edu.kz/handle/123456789/9080
dc.language.isoen
dc.subjectmoving mirror trajectory
dc.subjectblack hole formation
dc.subject1+1D correspondence
dc.subjectBogolubov coefficients
dc.subjectquantum field in curved spacetime
dc.titleBlack Hole – Moving Mirror I: An Exact Correspondence
dc.typeArticle

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